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51. A new family of planets? 'Ocean-Planets'

52. The CHEOPS mission

53. The hot dayside and asymmetric transit of WASP-189 b seen by CHEOPS

54. SPIRou: NIR velocimetry and spectropolarimetry at the CFHT

55. COSMOGRAIL

57. CHEOPS launch in 2019! – Payload Capabilities and In-Orbit Commissioning Preview

58. The CORALIE survey for southern extrasolar planets. XVIII. Three new massive planets and two low-mass brown dwarfs at greater than 5 AU separation

59. ANDES, the high resolution spectrograph for the ELT: science goals, project overview, and future developments

60. The CORALIE survey for southern extrasolar planets

62. Consequences of spectrograph illumination for the accuracy of radial-velocimetry

63. Broadband near-infrared astronomical spectrometer calibration and on-sky validation with an electro-optic laser frequency comb

64. HARPS Gets New Fibres After 12 Years of Operations

65. ELT-HIRES, the high resolution spectrograph for the ELT : results from the Phase A study

66. The Next Generation Transit Survey (NGTS)

67. ELT-HIRES, the high resolution spectrograph for the ELT: results from the Phase A study

68. Synchronously-Driven Microresonator Solitons and Application in Astronomy

70. Microresonator Solitons for Astronomical Spectrometer Calibration

71. NGTS: Next Generation Transit Survey

76. NGTS: Next Generation Transit Survey

78. NGTS: Next Generation Transit Survey

79. The CORALIE survey for southern extrasolar planets

82. ELT-HIRES, the high resolution spectrograph for the ELT: results from the Phase A study

83. NGTS: a robotic transit survey to detect Neptune and Super-Earth mass planets

86. The CORALIE survey for southern extrasolar planets

87. The ESPRI project: astrometric exoplanet search with PRIMA

88. Narrow-angle astrometry with PRIMA

91. Higher-precision radial velocity measurements with the SOPHIE spectrograph using octagonal-section fibers

94. The ESPRI Project: differential delay lines for PRIMA

95. The ESPRI project: astrometric exoplanet search with PRIMA

97. Could we identify hot ocean-planets with CoRoT, Kepler and Doppler velocimetry?

98. PEGASE: a DARWIN/TPF pathfinder

99. The ESPRI Project: differential delay lines for PRIMA.

100. The ESPRI project: astrometric exoplanet search with PRIMA.

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